Neutron star photobombs baby star | Condominium photo of the day for Feb. 3, 2026

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The Sundarban The Sundarban A blurry swirl of blue and yellow and red gas are seen in this image with a bright dot of light in the center

The Very Excellent Telescope (VLT) latest caught this characterize of a planetary nebula, information superhighway hosting each a neutron star and younger stars.
(Image credit: ESO/J. Suherli et al.)

In astronomy, appearances would possibly maybe presumably well moreover be deceiving, especially ought to you could presumably well presumably be looking out at objects which would possibly maybe presumably well be each a ways-off and intricate. Gorgeous clouds of gasoline are often grouped below the to find-all time length “nebula,” but the processes that gentle them up would possibly maybe presumably well moreover be radically different.

A planetary nebula, for instance, marks the leisurely-lifestyles shedding of field subject by a sun-care for star. (It has nothing to perform with planets; the name comes from the object’s passing resemblance to a planet, as seen by means of early telescopes.) A stellar nursery alerts the reverse: the messy, full of life starting of a new star’s lifestyles. Untangling which memoir you could presumably well presumably be seeing often requires detailed measurements of how the gasoline is provocative and what it is made of.

What is it?

The VLT these days captured a characterize of an object acknowledged as Ve 7–27, which used to be long concept to be a planetary nebula. Nonetheless, because of this of of observations from the MUSE instrument, the characterize reveals that Ve 7–27 is de facto a quiet-forming baby star, serving to to resolve the debate.

The main clues came from the structure of Ve 7–27, as full of life jets studded with shining knots, moreover called “bullets,” are emanating from the structure — a hallmark of new child stars interacting violently with their environment.

“Instead of being the ‘last breath’ of a dying star, Ve 7-27 is a newborn one,” said Janette Suherli, a Ph.D. candidate at the College of Manitoba in Canada and first author of the stumble on that revealed this consequence, said in a observation.

The build is it?

Ve 7–27 is positioned round 4,500 gentle-years away and is section of the Vela Junior supernova remnant.

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The Sundarban A blurry swirl of blue and yellow and red gas are seen in this image with a bright dot of light in the center

Object Ve 7–27 is idea of as a younger star because of this of its jets of vitality being shot out into its atmosphere. (Image credit: ESO/J. Suherli et al.)Why is it improbable?

The characterize contains each stellar beginnings and endings, as end to the center of the characterize is a compact, yellowish-green smudge that hosts a neutron star, the ultra-dense remnant left at the aid of when an enormous star exploded as a supernova. This build belongs to the Vela Junior supernova remnant, section of a broader cloud of field subject launched outward by that extinct explosion.

With the wait on of MUSE’s observations, astronomers chanced on that Ve 7–27 is embedded internal the field subject expelled by the Vela Junior supernova, which hyperlinks the new child star with the particles of a stellar demise. The connection moreover helps to resolve an extended-operating be troubled: the distance of Vela Junior. By tying it to Ve 7–27, whose distance is acknowledged, astronomers can express Vela Junior round the identical distance of 4,500 gentle-years away, resolving inconsistencies about the remnant’s magnificent dimension, enlargement rate and age.

Have to learn more?

You would possibly maybe presumably well learn more about star formation and supernovas.

Kenna Hughes-Castleberry is the Stammer material Supervisor at Condominium.com. Formerly, she used to be the Science Communicator at JILA, a physics analysis institute. Kenna is moreover a contract science journalist. Her beats encompass quantum expertise, AI, animal intelligence, corvids, and cephalopods.

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